corner
corner

Phys. Rev. D 74, 084011 (2006) [5 pages]

Gravitational diffraction radiation

Download: PDF (224 kB) Buy this article Export: BibTeX or EndNote (RIS)

Vitor Cardoso*
Department of Physics and Astronomy, University of Mississippi, University, Mississippi 38677-1848, USA

Marco Cavaglià
Department of Physics and Astronomy, University of Mississippi, University, Mississippi 38677-1848, USA

Mário Pimenta
Departamento de Física, IST, Avenida Rovisco Pais, 1049-001 Lisboa, Portugal
LIP, Avenida Elias Garcia, 14-1, 1000-149 Lisboa, Portugal

Received 9 August 2006; published 9 October 2006

We show that if the visible universe is a membrane embedded in a higher-dimensional space, particles in uniform motion radiate gravitational waves because of spacetime lumpiness. This phenomenon is analogous to the electromagnetic diffraction radiation of a charge moving near to a metallic grating. In the gravitational case, the role of the metallic grating is played by the inhomogeneities of the extra-dimensional space, such as a hidden brane. We derive a general formula for gravitational diffraction radiation and apply it to a higher-dimensional scenario with flat compact extra dimensions. Gravitational diffraction radiation may carry away a significant portion of the particle’s initial energy. This allows to set stringent limits on the scale of brane perturbations. Physical effects of gravitational diffraction radiation are briefly discussed.

© 2006 The American Physical Society

URL:
http://link.aps.org/doi/10.1103/PhysRevD.74.084011
DOI:
10.1103/PhysRevD.74.084011
PACS:
04.30.−w, 04.50.+h, 11.25.Wx

*Electronic address: vcardoso@phy.olemiss.edu

Electronic address: cavaglia@phy.olemiss.edu

Electronic address: pimenta@lip.pt

§Also at Centro de Física Computacional, Universidade de Coimbra, P-3004-516 Coimbra, Portugal